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  • Rule: ActivityStreamsMapasEquivalentb3sb3sifpdbprdf-labelfacetshttp://dbpedia.org/resource/inference/rules/dbpedia#http://dbpedia.org/resource/inference/rules/opencyc#http://dbpedia.org/resource/inference/rules/umbel#http://dbpedia.org/resource/inference/rules/yago#http://dbpedia.org/schema/property_rules#http://www.ontologyportal.org/inference/rules/SUMO#http://www.ontologyportal.org/inference/rules/WordNet#http://www.w3.org/2002/07/owl#ldpoplwebskos-transurn:det:rdf:labelvirtrdf-labelvirtrdf-urlNone
    
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About: 1647 Menelaus     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : umbel-rc:Planet, within Data Space : dbpedia.org associated with source document(s)

Type: Thingplacedbo:Locationschema:Placecelestial bodyPlanetyago:WikicatAsteroidsNamedFromGreekMythologyyago:WikicatAstronomicalObjectsDiscoveredIn1957yago:Asteroid109208702yago:CelestialBody109239740yago:MinorPlanet109355623yago:NaturalObject100019128yago:Object100002684yago:PhysicalEntity100001930yago:Planet109394007planetyago:Whole100003553umbel-rc:Planet New Facet based on Instances of this Class

1647 Menelaus /mɛnəˈleɪəs/ is a mid-sized Jupiter trojan from the Greek camp, approximately 42 kilometers (26 miles) in diameter. It was discovered on 23 June 1957 by American astronomer Seth Nicholson at the Palomar Observatory in California, and later named after the Spartan King Menelaus from Greek mythology. The dark asteroid has a rotation period of 17.7 hours. It is the principal body of the proposed , which encompasses several, mostly tentative Jovian asteroid families.